Wanted! Nuclear Data for Dark Matter Astrophysics

TL;DR

This paper emphasizes the critical need for improved nuclear data, such as cross sections and nucleon spin densities, to enhance dark matter detection methods and interpret cosmic ray measurements accurately.

Contribution

It highlights the importance of acquiring more precise nuclear physics data to reduce uncertainties in dark matter searches and cosmic ray modeling.

Findings

Current uncertainties hinder dark matter detection accuracy.

Better nuclear data can improve cosmic ray flux modeling.

Enhanced measurements could clarify observed excesses.

Abstract

Astronomical observations from small galaxies to the largest scales in the universe can be consistently explained by the simple idea of dark matter. The nature of dark matter is however still unknown. Empirically it cannot be any of the known particles, and many theories postulate it as a new elementary particle. Searches for dark matter particles are under way: production at high-energy accelerators, direct detection through dark matter-nucleus scattering, indirect detection through cosmic rays, gamma rays, or effects on stars. Particle dark matter searches rely on observing an excess of events above background, and a lot of controversies have arisen over the origin of observed excesses. With the new high-quality cosmic ray measurements from the AMS-02 experiment, the major uncertainty in modeling cosmic ray fluxes is in the nuclear physics cross sections for spallation and fragmentation of cosmic rays off interstellar hydrogen and helium. The understanding of direct detection backgrounds is limited by poor knowledge of cosmic ray activation in detector materials, with order of magnitude differences between simulation codes. A scarcity of data on nucleon spin densities blurs the connection between dark matter theory and experiments. What is needed, ideally, are more and better measurements of spallation cross sections relevant to cosmic rays and cosmogenic activation, and data on the nucleon spin densities in nuclei.